Ion-atom complexes and the absorption of radiation in stellar plasma
1992
In order to provide the relevant absorption coefficients for the interpretation of the continuum absorption spectra in stellar atmospheres, the processes H 2 + + hw → H + H+ and H + H + hw → H + H+ have been considered together, as well as the same processes in the helium case. We present here the corresponding coefficients for the conditions of stellar atmospheres.
Keywords:
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
2
References
0
Citations
NaN
KQI